Cosmic Ray rejection with attention augmented deep learning

نویسندگان

چکیده

Cosmic Ray (CR) hits are the major contaminants in astronomical imaging and spectroscopic observations involving solid-state detectors. Correctly identifying masking them is a crucial part of image processing pipeline, since it may otherwise lead to spurious detections. For this purpose, we have developed tested novel Deep Learning based framework for automatic detection CR from data two different imagers: Dark Energy Camera (DECam) Las Cumbres Observatory Global Telescope (LCOGT). We considered baseline models namely deepCR Cosmic-CoNN, which current state-of-the-art learning algorithms that were trained using Hubble Space (HST) ACS/WFC LCOGT Network images respectively. experimented with idea augmenting Attention Gates (AGs) improve performance. our on DECam demonstrate consistent marginal improvement by adding AGs True Positive Rate (TPR) at 0.01% False (FPR) Precision 95% TPR over aforementioned dataset. proposed AG augmented provide significant gain FPR when previously unseen LCO test having three distinct telescope classes. Furthermore, without attention augmentation outperform such as Astro-SCRAPPY, Maximask (that natively data) pre-trained ground-based Cosmic-CoNN. This study demonstrates module enables us get better Cosmic-CoNN their generalization capability data.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Cosmic Ray Rejection in STIS CCD Images

We describe the method of noise model-based cosmic ray (CR) rejection in multiple, registered images, and discuss its implementation in the context of the STIS calibration pipeline. We focus on the method by which the various contributions to the uncertainty in the final, calibrated image should be combined. Unfortunately, the current design of the CR rejection module, calstis2, makes it diffic...

متن کامل

Memory-Efficient Up-the-Ramp Processing with Cosmic-Ray Rejection

We introduce a memory-efficient method for processing up-the-ramp sampled data to reduce noise and remove cosmic-ray events. The method we describe includes initial processing in the readout electronics (onboard, in the case of a space mission) plus postprocessing downstream. This data processing approach can be used to record or downlink high-quality science data using a small fraction of the ...

متن کامل

Time Delays in Cosmic Ray Propagation

Cosmic Rays (CR) travel at speeds essentially indistinguishable from the speed of light. However whilst travelling through magnetic fields, both regular and turbulent, they are delayed behind the light since they are usually charged particles and their paths are not linear. Those delays can be so long that they are an impediment to correctly identifying sources which may be variable in time. Fu...

متن کامل

Calstis2: Cosmic Ray Rejection in the STIS Calibration Pipeline

We describe calstis2, the calstis calibration module which combines CRSPLIT and repeated exposures to produce a single, cosmic ray rejected image. Cosmic ray rejection in the STIS pipeline employs a noise model and parameterized rejection criteria to identify and exclude discrepant values in forming the output image. The calstis pipeline is able to perform this cosmic ray rejection because the ...

متن کامل

The STScI STIS Pipeline V: Cosmic Ray Rejection

In this ISR we describe calstis-2, the calstis calibration module which combines CRSPLIT exposures to produce a single cosmic ray rejected image. Cosmic ray rejection in the STIS pipeline will follow the same basic philosophy as does the STSDAS task crrej a series of separate CRSPLIT exposures are combined to produce a single summed image, where discrepant (different by some number of sigma fro...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Astronomy and Computing

سال: 2022

ISSN: ['2213-1345', '2213-1337']

DOI: https://doi.org/10.1016/j.ascom.2022.100625